Electrification of sand on Titan and its influence on sediment transport
Autor: | George D. McDonald, Devon M. Burr, Michael Malaska, J. S. Méndez Harper, Josef Dufek, J. McAdams, James J. Wray, Alexander G. Hayes |
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Rok vydání: | 2017 |
Předmět: |
geography
Solar System geography.geographical_feature_category 010504 meteorology & atmospheric sciences Granular material 01 natural sciences Astrobiology symbols.namesake Volcano Saltation (geology) 0103 physical sciences symbols General Earth and Planetary Sciences Titan (rocket family) 010303 astronomy & astrophysics Sediment transport Geomorphology Geology Magnetosphere particle motion Triboelectric effect 0105 earth and related environmental sciences |
Zdroj: | Nature Geoscience. 10:260-265 |
ISSN: | 1752-0908 1752-0894 |
DOI: | 10.1038/ngeo2921 |
Popis: | Triboelectric, or frictional, charging is a ubiquitous yet poorly understood phenomenon in granular flows. Recognized in terrestrial volcanic plumes and sand storms, such electrification mechanisms are possibly present on Titan. There, dunes and plains of low-density organic particles blanket extensive regions of the surface. Unlike Earth, Titan hosts granular reservoirs whose physical and chemical properties possibly enhance the effects of charging on particle motion. Here we demonstrate in laboratory tumbler experiments under atmospheric conditions and using organic materials analogous to Titan that Titan sands can readily charge triboelectrically. We suggest that the resulting electrostatic forces are strong enough to promote aggregation of granular materials and affect sediment transport on Titan. Indeed, our experiments show that electrostatic forces may increase the saltation threshold for grains by up to an order of magnitude. Efficient electrification may explain puzzling observations on Titan such as the mismatch between dune orientations and inferred wind fields. We conclude that, unlike other Solar System bodies, nanometre-scale electrostatic processes may shape the geomorphological features of Titan across the moon’s surface. Frictional charging of granular materials may readily occur on Saturn’s moon Titan. Laboratory experiments under Titan-like conditions suggest that the resulting electrostatic forces are strong enough to affect sand transport on Titan. |
Databáze: | OpenAIRE |
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